The sun has a radius of 6.959 × 108 m and a surface temperature of 5.81 x 10° K.When the sun radiates at a rate of 3.91 x 1026 W and is a perfect emitter. What isthe rate of energy emitted per square meter? Stefan-Boltzmann constant is 5.67 x10-8 J/s-m2 K4a)5.6 x 107 W/m2b) 12.8 x 107 W/m2c)6.4 x 107 W/m225.6 x 107 W/m25.6 x 1017 W/m2

Given r=6.959×108 mT=5.81×103 KQ=3.91×1026 Wσ=5.67×10-8 J/s *m2K4

The sun has a radius of 6.959 x 10° m and a surface temperature of When the sun radiates at a rate of 3.91 x 1026 W and is a perfect er the rate of energy emitted per square meter? Stefan-Boltzmann co 10-8 /s-m2 K4

The sun has a radius of 6.959 x 10° m and a surface temperature of When the sun radiates at a rate of 3.91 x 1026 W and is a perfect er the rate of energy emitted per square meter? Stefan-Boltzmann co 10-8 /s-m2 K4

College Physics

11th Edition

ISBN:9781305952300

Author:Raymond A. Serway, Chris Vuille

Publisher:Raymond A. Serway, Chris Vuille

Chapter1: Units, Trigonometry. And Vectors

Section: Chapter Questions

Problem 1CQ: Estimate the order of magnitude of the length, in meters, of each of the following; (a) a mouse, (b)...

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Concept explainers

Wien's displacement law

Students often get confused between Wien's displacement law and Planck's radiation law. Although both are historically related, yet they are conceptually different. Planck's law helps determine the spectrum of a blackbody, while Wien's law determines the relationship between peak wavelength and temperature.

Question

The sun has a radius of 6.959 × 108 m and a surface temperature of 5.81 x 10° K.
When the sun radiates at a rate of 3.91 x 1026 W and is a perfect emitter. What is
the rate of energy emitted per square meter? Stefan-Boltzmann constant is 5.67 x
10-8 J/s-m2 K4
a)
5.6 x 107 W/m2
b) 12.8 x 107 W/m2
c)
6.4 x 107 W/m2
25.6 x 107 W/m2
5.6 x 1017 W/m2

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